We release a data set to accompany the paper "Event Horizon Telescope observations of the jet launching and collimation in Centaurus A) (Janssen et al. 2021; DOI: https://doi.org/10.1038/s41550-021-01417-w). These data are the calibrated visibilities from the Event Horizon Telescope observations of Centaurus A from April 10, 2017 for both "low" and "high" bands, centred around 227.1 GHz and 229.1 GHz, respectively. Data from the 2017 observations were processed through three independent reduction pipelines (Blackburn et al. 2019, Janssen et al. 2019, EHTC et al. 2019). This release includes the fringe fitted, a-priori calibrated, and network calibrated "casa" and "hops" data from the rPICARD and EHT-HOPS pipelines, respectively. Independent flux calibration is performed based on estimated station sensitivities during the campaign (Issaoun et al. 2017, Janssen et al. 2019). A description of the data properties, their validation, and estimated systematic errors is given in EHTC et al. (2019) with additional details in Wielgus et al. (2019). The data are time averaged to 10 seconds and frequency averaged over all 32 intermediate frequencies (IFs). All polarization information is explicitly removed. To make the resulting "uvfits" files compatible with popular very-long-baseline interferometry (VLBI) software packages, the circularly polarized cross-hand visibilities RL and LR are set to zero along with their errors, while parallel-hands RR and LL are both set to an estimated Stokes I value. Measurement errors for RR and LL are each set to sqrt(2) times the statistical errors for Stokes I.